Paper Citation Record · LEDGER

Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1504.01266.

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pith.paper-citation-record.v1
1504.01266 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:25:17.456488Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-09T20:06:29.644846Z

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Outbound references

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Pith citing papers

Observation bda0fae0-5471-4575-b368-7ae93b6248cf · inbound

Matter And Gravitation In Collisions of heavy ions and neutron stars: equation of state cites this paper.

Matter And Gravitation In Collisions of heavy ions and neutron stars: equation of state Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-05-24T22:15:00.828104Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 5189230f-4b48-4937-ab44-79bc23b5a12d · inbound

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity cites this paper.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.629131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4ed2abf-1f86-4431-8c71-75a2f04963ff · inbound

Rotating neutron stars with non-barotropic thermal profile cites this paper.

Rotating neutron stars with non-barotropic thermal profile Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-14T10:30:45.111585Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45f76b3f-90da-416b-b620-8255911e5c9a · inbound

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter cites this paper.

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-14T10:20:11.717252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5778f0a-eedc-4a5a-9cbe-d427f5ad8439 · inbound

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung cites this paper.

Cooling binary neutron star remnants via nucleon-nucleon-axion bremsstrahlung Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-14T05:28:09.053614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf8a0b2d-e965-48a5-a049-f6f8ba5240a6 · inbound

Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme cites this paper.

Eccentricity reduction of binary neutron star initial data with the entropy based flux limiting scheme Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-11T10:51:21.687842Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ccb3ed28-cc4a-4fdc-966c-2a9839abcca2 · inbound

Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars cites this paper.

Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-16T05:25:17.456488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 61cd3302-039f-447e-b6ac-f6bdea3c1e23 · inbound

The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.

The error budget of binary neutron star merger simulations for configurations with high spin Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 151

Resolution: unresolved; no resolver link, observed 2026-08-07T11:41:09.879682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7f712a3-5b16-49fb-ac14-99f5f94b38e0 · inbound

Exact Mass Conservation in Binary Neutron Star Merger Simulations cites this paper.

Exact Mass Conservation in Binary Neutron Star Merger Simulations Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-06-29T05:53:09.162092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 4b95247b-ce4c-4fe5-8fd6-4e04ba9fd819 · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 148

Resolution: verified exact; local_arxiv, observed 2026-07-09T20:06:29.646229Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.